First results from the CRESST-III low-mass dark matter program

被引：348

作者：

Abdelhameed, A. H. ^{[1
]}

Angloher, G. ^{[1
]}

Bauer, P. ^{[1
]}

Bento, A. ^{[1
,9
]}

Bertoldo, E. ^{[1
]}

Bucci, C. ^{[2
]}

Canonica, L. ^{[1
]}

D'Addabbo, A. ^{[2
,10
]}

Defay, X. ^{[3
,4
]}

Di Lorenzo, S. ^{[2
,10
]}

Erb, A. ^{[3
,4
,11
]}

Feilitzsch, F. v ^{[3
,4
]}

Fichtinger, S. ^{[5
]}

Iachellini, N. Ferreiro ^{[1
]}

Fuss, A. ^{[5
,6
]}

Gorla, P. ^{[2
]}

Hauff, D. ^{[1
]}

Jochum, J. ^{[7
]}

Kinast, A. ^{[3
,4
]}

Kluck, H. ^{[5
,6
]}

Kraus, H. ^{[8
]}

Langenkaemper, A. ^{[3
,4
]}

Mancuso, M. ^{[1
]}

Mokina, V ^{[5
]}

Mondragon, E. ^{[3
,4
]}

Muenster, A. ^{[3
,4
]}

Olmi, M. ^{[2
,10
]}

Ortmann, T. ^{[3
,4
]}

Pagliarone, C. ^{[2
,12
]}

Pattavina, L. ^{[3
,4
,10
]}

Petricca, F. ^{[1
]}

Potzel, W. ^{[3
,4
]}

Proebst, F. ^{[1
]}

Reindl, F. ^{[5
,6
]}

Rothe, J. ^{[1
]}

Schaffner, K. ^{[2
,10
]}

Schieck, J. ^{[5
,6
]}

Schipperges, V ^{[7
]}

Schmiedmayer, D. ^{[5
,6
]}

Schoenert, S. ^{[3
,4
]}

Schwertner, C. ^{[5
,6
]}

Stahlberg, M. ^{[5
,6
]}

Stodolsky, L. ^{[1
]}

Strandhagen, C. ^{[7
]}

Strauss, R. ^{[3
,4
]}

Tuerkoglu, C. ^{[5
,6
]}

Usherov, I ^{[7
]}

Willers, M. ^{[3
,4
]}

Zema, V ^{[2
,10
,13
]}

机构：

[1] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[2] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Assergi, Italy

[3] Tech Univ Munich, Phys Dept, D-85747 Garching, Germany

[4] Tech Univ Munich, Excellence Cluster Universe, D-85747 Garching, Germany

[5] Austrian Acad Sci, Inst Hochenergiephys, A-1050 Vienna, Austria

[6] Tech Univ Wien, Atominst, A-1020 Vienna, Austria

[7] Eberhard Karts Univ Tubingen, D-72076 Tubingen, Germany

[8] Univ Oxford, Dept Phys, Oxford OX1 3RH, England

[9] Univ Coimbra, Dept Fis, LIBPhys, P-3004516 Coimbra, Portugal

[10] Gran Sasso Sci Inst, I-67100 Laquila, Italy

[11] Walther Meissner Inst Tieftemp Forsch, D-85748 Garching, Germany

[12] Univ Cassino & Lazio Meridionale, Dipartimento Ingn Civile & Meccan, I-03043 Cassino, Italy

[13] Chalmers Univ Technol, Dept Phys, S-41296 Gothenburg, Sweden

来源：

PHYSICAL REVIEW D | 2019年 / 100卷 / 10期

关键词：

SEARCH; SCATTERING; DETECTORS;

D O I：

10.1103/PhysRevD.100.102002

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The CRESST experiment is a direct dark matter search which aims to measure interactions of potential dark matter particles in an Earth-bound detector. With the current stage, CRESST-III, we focus on a low energy threshold for increased sensitivity towards light dark matter particles. In this paper we describe the analysis of one detector operated in the first run of CRESST-III (05/2016-02/2018) achieving a nuclear recoil threshold of 30.1 eV. This result was obtained with a 23.6 g CaWO4 crystal operated as a cryogenic scintillating calorimeter in the CRESST setup at the Laboratori Nazionali del Gran Sasso (LNGS). Both the primary phonon (heat) signal and the simultaneously emitted scintillation light, which is absorbed in a separate silicon-on-sapphire light absorber, are measured with highly sensitive transition edge sensors operated at similar to 15 mK. The unique combination of these sensors with the light element oxygen present in our target yields sensitivity to dark matter particle masses as low as 160 MeV/c(2).

引用

页数：11

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